A dataset provided by the European Space Agency

Proposal ID 050616
Title Simultaneous observations of the X-ray and IR flares of GRS 1915+105
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506160901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506161001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506161101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506161201

DOI https://doi.org/10.5270/esa-xu6je85
Principal Investigator, PI Dr Gloria Sala
Abstract GRS 1915+105 is the most prominent microquasar and the most energetic object inour Galaxy. It has remained unique among its class for the large variety oftemporal behaviours in different time scales. Multiwavelength observationsshowing radio, IR and X-ray oscilations, with time delays depending on thewavelength, revealed in the past the intimate link between the accretion discand the jet ejection. However, the mechanism of jet formation and the origin ofthe delay between the flares in different wavelengths remains unclear. Here wepropose simultaneous X-ray and IR observations of GRS 1915+105 withunprecedented high time resolution, using EPIC-pn in Burst mode and VLT/ISAAC.sAladdin array in its new Burst mode, with integration times as short as 3.2ms.
Publications
Instrument EPN, RGS1, RGS2
Temporal Coverage 2007-09-24T00:17:11Z/2007-09-30T05:59:44Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2008-11-14T00:00:00Z
Keywords "jet ejection", "aladdin array", "EPIC", "burst mode", "time resolution", "time scales", "accretion disc", "xray oscilations", "time delays depending", "jet formation", "epic pn", "prominent microquasar", "intimate link", "temporal behaviours", "energetic object", "grs 1915"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Gloria Sala, 2008, 'Simultaneous observations of the X-ray and IR flares of GRS 1915+105', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xu6je85